Перегляд архіву четвер, 23 жовтня 2014

Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2014 Oct 23 1257 UTC

Прогноз SIDC

Сонячні спалахи

Major flares expected (X-class flares expected, probability >=50%)

Геомагнетизм

Quiet (A<20 and K<4)

Сонячні протони

Warning condition (activity levels expected to increase, but no numeric forecast given)

	10 см потік	Ap
23 Oct 2014	221	012
24 Oct 2014	226	012
25 Oct 2014	231	011

Бюлетень

During the past 24 hours, Catania sunspot group 88 (NOAA AR 2192) produced an X1.6 flare (peaking yesterday at 14:28 UT) and an M1.1 flare (peaking today at 09:50 UT). These flares were not associated with CMEs. Catania sunspot group 93 (NOAA AR 2195) close to the east solar limb produced an M1.4 flare peaking at 15:57 UT, and this flare was associated only with a narrow CME. Catania sunspot group 88 will remain the main flare source as it continues to grow (this is the largest sunspot group during the two solar cycles) and maintains the beta-gamma-delta configuration of its photospheric magnetic field. Although the sunspots of the main magnetic polarities are somewhat separating, we still expect the flaring activity up to X-level from this sunspot group. As the Catania sunspot group 88 is currently situated at the solar central meridian, a major eruption in this active region may lead to a geoeffective CME and a proton event. The Earth is currently inside a slow (around 430 km/s) solar wind flow with average (around 5 nT) interplanetary magnetic field (IMF) magnitude. The geomagnetic conditions are quiet and are expected to remain so. Yesterday an interval of K = 5 was reported by IZMIRAN and an interval of K = 4 by Dourbes (K index according to NOAA remained at the quiet to unsettled levels with K < 4). This interval of slightly disturbed geomagnetic conditions was produced by a slow solar wind interval with predominantly negative north-south IMF component Bz.

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 091, за даними 05 станцій.

Сонячні індекси за 22 Oct 2014

Число Вольфа, Катанія	202
Сонячний потік 10 см	216
AK Chambon La Forêt	///
AK Wingst	///
Розрахунковий індекс Ap	017
Розрахункова міжнародна кількість сонячних плям	098 - За даними 16 станцій

Зведення помітних подій

Надано Центром Аналізу Даних Сонячного Впливу (SIDC)© - SIDC - Оброблено SpaceWeatherLive

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